HI observations of dwarf galaxies out to a distance of 50 MPC

Details HI observations of dwarf galaxies out to a distance of 50 MPC HI observations of dwarf galaxies out to a distance of 50 MPC

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..181s&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 181-182 (SEE N93-26706 10-90)

Physics

Distance, Dwarf Galaxies, Galactic Clusters, Stellar Mass, Hydrogen, Sensitivity, Star Formation

Scientific paper

Here we report our preliminary findings from an HI search for dwarf galaxies in three environmentally distinct regions of the sky: a galactic void, a galactic cluster, and an interaction field. This study is sensitive at the 5(sigma) level to hydrogen masses as low as 5 x 10(exp 5) solar mass. We have made three possible detections of previously uncatalogued objects: one in the void field, and two in the cluster field. Reduction of the interaction field is in progress.

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